\begin{table}%t2 \par \protect\caption{\label{obslog}New near-infrared observations$^a$.} %\centerline { \begin{tabular}{c c c c c c c c c c} \hline\hline ID & $\alpha$~~~~~~~~~~~~~~~~~~~~~~~~~~~~$\delta$ & Instr. & Filter & Area & Date(s) & $t_{\rm exp}$ & $m_{\rm cmp}$ & $m_{\rm lim}$ \\ & (J2000)~~~~~~~~~~~~~(J2000) &&& (arcmin$^2$)&& (min) & (mag) & (mag) \\ \hline 1-k & 05 39 39.9 ~~~$-$02 50 26 & Omega2000 & $K_{\rm s}$ &197 (279)& 2005 Jan. 31, Feb. 1, Oct. 26& 326 & 20.5 & 21.2 \\ 2-j & 05 39 35.1 ~~~$-$02 34 44 & Omega2000 & $J$ &214 (259)& 2006 Oct. 07 & 63 & 20.9 & 21.9 \\ 2-h & 05 39 19.3 ~~~$-$02 33 36 & Omega2000 & $H$ &181 (295)& 2005 Oct. 19 & 186 & 21.2 & 21.9 \\ 2-k & 05 39 21.2 ~~~$-$02 35 14 & Omega2000 & $K_{\rm s}$ &194 (282)& 2005 Oct. 24--25 & 139.5 & 20.1 & 21.0 \\ 3-h & 05 38 40.1 ~~~$-$02 48 09 & SofI & $H$ & 21 (27) & 2006 Dec. 27 & 147 & 20.3 & 20.9 \\ 4-h & 05 38 40.0 ~~~$-$02 52 26 & SofI & $H$ & 21 (27) & 2006 Dec. 24 & 98 & 20.3 & 21.1 \\ 5-h & 05 38 39.7 ~~~$-$02 57 09 & SofI & $H$ & 21 (27) & 2006 Dec. 27 & 75 & 20.1 & 20.5 \\ 6-h & 05 38 20.0 ~~~$-$02 48 30 & SofI & $H$ & 21 (27) & 2006 Dec. 24 & 201 & 20.1 & 21.1 \\ 7-h & 05 40 05.1 ~~~$-$02 30 40 & SofI & $H$ & 21 (27) & 2006 Dec. 27 & 132 & 20.3 & 21.1 \\ 8-h & 05 40 04.9 ~~~$-$02 35 57 & SofI & $H$ & 21 (27) & 2006 Dec. 26 & 98 & 19.5 & 20.1 \\ 9-h & 05 40 03.6 ~~~$-$02 42 10 & SofI & $H$ & 21 (27) & 2006 Dec. 25 & 56 & 19.9 & 20.7 \\ 10-h & 05 39 09.7 ~~~$-$02 47 15 & SofI & $H$ & 21 (27) & 2006 Dec. 25 & 168 & 20.3 & 21.3 \\ 11-h & 05 39 27.7 ~~~$-$02 47 15 & SofI & $H$ & 21 (27) & 2006 Dec. 25 & 95 & 20.1 & 21.1 \\ 12-h & 05 39 45.7 ~~~$-$02 47 15 & SofI & $H$ & 21 (27) & 2006 Dec. 26 & 120 & 20.3 & 21.3 \\ 13-h & 05 40 03.1 ~~~$-$02 47 04 & SofI & $H$ & 16 (33) & 2006 Dec. 26 & 140 & 20.3 & 21.1 \\ 14-h & 05 39 09.5 ~~~$-$02 53 56 & LIRIS & $H$ & 16 (20) & 2006 Dec. 29 & 36 & 19.5 & 20.1 \\ 15-h & 05 39 45.4 ~~~$-$02 53 57 & LIRIS & $H$ & 16 (20) & 2007 Dec. 14 & 45 & 20.3 & 20.9 \\ 16-h & 05 40 03.6 ~~~$-$02 53 59 & LIRIS & $H$ & 16 (20) & 2007 Dec. 14 & 45 & 20.3 & 20.9 \\ \hline \end{tabular}} \par \smallskip $^a$ Fields of view (and pixel scales) of the Omega2000, SofI, and LIRIS detectors are $15.4\times15.4$~arcmin$^2$ (0.45~arcsec~${\rm pixel}^{-1}$), $4.9\times4.9$~arcmin$^2$ (0.288~arcsec~${\rm pixel}^{-1}$), and $4.2\times4.2$~arcmin$^2$ (0.25~arcsec~${\rm pixel}^{-1}$), respectively. \end{table}